{"id":714,"date":"2007-07-19T09:33:56","date_gmt":"2007-07-19T06:33:56","guid":{"rendered":"http:\/\/www.fyysika.ee\/wordpress\/?p=714"},"modified":"2010-03-29T09:58:50","modified_gmt":"2010-03-29T06:58:50","slug":"chandra-lahendab-musta-augu-musteeriumi","status":"publish","type":"post","link":"https:\/\/www.fyysika.ee\/?p=714","title":{"rendered":"Chandra lahendab musta augu m\u00fcsteeriumi"},"content":{"rendered":"<div style=\"text-align: justify;\"><span style=\"font-weight: bold;\">See, kuidas mustad augud imevad sisse mateeriat naaberalade t\u00e4htedelt, on fundamentaalselt magneetiline protsess ning mitte ainult gravitatsioonist p\u00f5hjustatud. Sellisele j\u00e4reldusele j\u00f5uti t\u00e4nu uutele m\u00f5\u00f5tmistele, mis tehti r\u00f6ntgenkiirgust kiirgavast, gaasist \u00fcmbritsetud mustast august Linnuteel. Kuigi teooria ennustas seda juba 30 aastat tagasi, on n\u00fc\u00fcd esimene kord, kui seda efekti n\u00e4ha saab. Chandra r\u00f6ntgenkiirte observatooriumi m\u00f5\u00f5tmistel  p\u00f5hinevad tulemused v\u00f5ivad m\u00f5jutada teooriaid selle kohta, kuidas mateeria imetakse musta auku v\u00f5i teiste kompaktsete objektide kohta. (<\/span><i style=\"font-weight: bold;\">Nature 441 953<\/i><span style=\"font-weight: bold;\">).<\/span><\/div>\n<p>Mustadel aukudel on nii tugev gravitatsiooniv\u00e4li, et <\/p>\n<table rules=\"none\" frame=\"void\" cellspacing=\"1\" cellpadding=\"10\" border=\"0\" align=\"right\" style=\"border-style: none; width: 296px; height: 250px; background-image: none; float: right; text-align: left; vertical-align: top;\">\n<tbody>\n<tr>\n<td><font size=\"2\"><img decoding=\"async\" hspace=\"0\" border=\"0\" align=\"bottom\" src=\"pildid\/mauk1.jpg\" \/><\/font><\/td>\n<\/tr>\n<tr style=\"font-style: italic;\">\n<td><font size=\"2\">Musta augu r\u00f6ntgenspekter (all paremal) &#8211; allikas Michigani \u00fclikool<\/font><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p><font size=\"2\">nad t\u00f5mbavad k\u00fclge suures koguses naaberalade gaasi ja tolmu. See mateeria moodustab \u201ejuurdekasvu-ketta\u201c (&quot;<i>accretion disk<\/i>&quot;) \u00fcmber augu nagu r\u00f5ngad \u00fcmber Saturni. H\u00f5\u00f5rdej\u00f5ud ketta kokkusurumisel p\u00f5rkuvate mateeria osakeste vahel paneb selle kuumenema ning r\u00f6ntgenkiirgust emiteerima. Seda on aga astronoomidel v\u00f5imalik avastada ning nad saavad korjata vaatlusel p\u00f5hinevaid t\u00f5endeid mustade aukude kohta.<\/font><\/p>\n<p align=\"justify\" style=\"margin: 0cm 0cm 6pt;\" class=\"MsoNormal\"><span lang=\"ET\"><font size=\"2\">Sellegi poolest on astronoomid juba pikalt m\u00f5istnud, et gravitatsioonist \u00fcksi ei piisa gaasi imemiseks musta auku. Enne kui gaas saab sisse spiraliseeruda, peab ta kaotama osa oma nurkmomendist. Vastupidisel juhul j\u00e4\u00e4ks see m\u00e4\u00e4ramatult orbiidile \u00fcmber musta augu. <br \/><\/font><\/span><\/p>\n<p align=\"justify\" style=\"margin: 0cm 0cm 6pt;\" class=\"MsoNormal\"><span lang=\"ET\"><\/span><span lang=\"ET\"><font size=\"2\">Senini ei olnud kindel, kuidas see nurkmoment eemaldati, kuid teadlased kahtlustasidmagneetilist turbulentsi kettas. Turbulents genereerib h\u00f5\u00f5rdumist kettas ning juhib tuult eemale. Tuul p\u00f5hjustab nurkmomendi v\u00e4henemist ning lubab mateerial musta auku kukkuda.<br \/><\/font><\/span><\/p>\n<p align=\"justify\" style=\"margin: 0cm 0cm 6pt;\" class=\"MsoNormal\"><span lang=\"ET\"><\/span><span lang=\"ET\"><font size=\"2\">Jon Miller Michigani \u00dclikoolist ja tema kolleegid on n\u00fc\u00fcdseks toonud esimese vaatlusel p\u00f5hineva t\u00f5endi,<\/font><\/span><font size=\"2\"> et magnetv\u00e4ljad t\u00f5esti tekitavad sellist efekti. Meeskond uuris t\u00e4he massiga musta auku GRO J1655-40<span style=\"color: blue;\">&nbsp;<\/span>Linnuteel, kasutades selleks NASA Chandra r\u00f6ntgenkiirguse observatooriumit. <\/font><span lang=\"ET\"><font size=\"2\">&nbsp;<\/font><\/p>\n<table rules=\"none\" frame=\"void\" cellspacing=\"1\" cellpadding=\"10\" border=\"0\" align=\"left\" style=\"border-style: none; width: 30%; background-image: none; float: left; text-align: left; vertical-align: top;\">\n<tbody>\n<tr>\n<td><font size=\"2\"><img decoding=\"async\" hspace=\"0\" border=\"0\" align=\"bottom\" src=\"pildid\/mauk2.jpg\" \/><\/font><\/td>\n<\/tr>\n<tr>\n<td><font size=\"2\"><span style=\"font-style: italic;\">Kunstniku n\u00e4gemus musta augu magnetv\u00e4lja m\u00f5just &#8211; allikas Michigani \u00fclikool<\/span><\/font><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p><\/span><font size=\"2\">GRO J1655-40 on ainult 10 000 v.a. kaugusel. R\u00f6ngenkiirguse spekter mustast august n\u00e4itab, et tuule kiirus ja tihedus J1655\u2019e kettal vastavad teoreetilistele simulatsioonidele, mida meeskond esitas magneetiliselt juhitud tuulte kohta.<\/font><\/p>\n<p align=\"justify\" style=\"margin: 0cm 0cm 6pt;\" class=\"MsoNormal\"><span lang=\"ET\"><font size=\"2\">Vastavalt Millerile ja ta kaaslastele v\u00f5ivad uued tulemused anda meile m\u00f5ista, kuidas mateeria langeb musta auku, kuidas augud kasvavad ning kuidas nad m\u00f5jutavad oma keskkonda. Nende t\u00f6\u00f6 v\u00f5ib samuti olla t\u00e4htis selgitamaks magnetv\u00e4ljade m\u00f5ju teiste kompaktsete objektide juurdekasvul nagu n\u00e4iteks neutront\u00e4hed ja valged k\u00e4\u00e4bused.<\/font><\/span><\/p>\n<p align=\"justify\" style=\"margin: 0cm 0cm 6pt;\" class=\"MsoNormal\"><span lang=\"ET\"><font size=\"2\">&nbsp;<\/font><\/p>\n<p \/><\/span><\/p>\n<p align=\"justify\" style=\"margin: 0cm 0cm 6pt;\" class=\"MsoNormal\"><span lang=\"ET\"><font size=\"2\">Allikas: <\/font><a href=\"http:\/\/physicsweb.org\/articles\/news\/10\/6\/10\/1#0606102\"><font size=\"2\">http:\/\/physicsweb.org\/articles\/news\/10\/6\/10\/1#0606102<\/font><\/a><\/span><\/p>\n<p align=\"justify\" style=\"margin: 0cm 0cm 6pt;\" class=\"MsoNormal\"><span lang=\"ET\"><font size=\"2\">Koostas: ALI<\/font><\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>See, kuidas mustad augud imevad sisse mateeriat naaberalade t\u00e4htedelt, on fundamentaalselt magneetiline protsess ning mitte ainult gravitatsioonist p\u00f5hjustatud. Sellisele j\u00e4reldusele j\u00f5uti t\u00e4nu uutele m\u00f5\u00f5tmistele, mis tehti r\u00f6ntgenkiirgust kiirgavast, gaasist \u00fcmbritsetud mustast august Linnuteel. Kuigi teooria ennustas seda juba 30 aastat tagasi, on n\u00fc\u00fcd esimene kord, kui seda efekti n\u00e4ha saab. Chandra r\u00f6ntgenkiirte observatooriumi m\u00f5\u00f5tmistel p\u00f5hinevad [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_genesis_hide_title":false,"_genesis_hide_breadcrumbs":false,"_genesis_hide_singular_image":false,"_genesis_hide_footer_widgets":false,"_genesis_custom_body_class":"","_genesis_custom_post_class":"","_genesis_layout":"","footnotes":""},"categories":[16],"tags":[],"class_list":{"0":"post-714","1":"post","2":"type-post","3":"status-publish","4":"format-standard","6":"category-teadusuudis","7":"entry"},"_links":{"self":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/posts\/714","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=714"}],"version-history":[{"count":0,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/posts\/714\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=714"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=714"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=714"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}